The State of the Art in Constraining Axion-to-Nucleon Coupling and Non-Newtonian Gravity from Laboratory Experiments
arXiv:2009.04517 · doi:10.3390/universe6090147
Abstract
Constraints on the Yukawa-type corrections to Newton's gravitational law and on the coupling constant of axionlike particles to nucleons obtained from different laboratory experiments are reviewed and compared. The constraints on non-Newtonian gravity under discussion cover the wide interaction range from nanometers to millimeters and follow from the experiments on neutron scattering, measuring the Casimir force and Cavendish-type experiments. The constraints on the axion-to-nucleon coupling constant following from the magnetometer measurements, Cavendish-type experiments, Casimir physics, and experiments with beams of molecular hydrogen are considered which refer to the region of axion masses from eV to 200 eV. Particular attention is given to the recent constraints obtained from measuring the Casimir force at nanometer separation distance between the test bodies. Several proposed experiments focused on constraining the non-Newtonian gravity, axionlike particles and other hypothetical weakly interacting particles, such as chameleons and symmetrons, are discussed.
21 pages, 10 figures; Special issue "Selected Papers from the 17th Russian Gravitational Conference -- International Conference on Gravitation, Cosmology and Astrophysics (RUSGRAV-17)"
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- Pendellösung Interferometry Probes the Neutron Charge Radius, Lattice Dynamics, and Fifth Forces
- From Supernovae to Neutron Stars: A Systematic Approach to Axion Production at Finite Density
- Gravitational Harmonium: Gravitationally Induced Entanglement in a Harmonic Trap
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- Leading bounds on micro- to picometer fifth forces from neutron star cooling
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